Optical Counterparts of Radio Pulsars (fos 38) Augmentation: Cycle 3 - High

Details Optical Counterparts of Radio Pulsars (fos 38) Augmentation: Cycle 3 - High Optical Counterparts of Radio Pulsars (fos 38) Augmentation: Cycle 3 - High

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.4863m&link_type=abstract

HST Proposal ID #4863

Physics

Hst Proposal Id #4863

Scientific paper

The FOS GTO program includes a systematic study of degenerate stars. FOS spectra of the Crab will be used to measure the spectral index (especially UV) of the nonthermal pulsar radiation, to verify synchrotron mechanism and search for spectral breaks. Absorption may be seen due to intervening gas, whose abundance and physical state could then be probed.

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